On the classic heat conduction in the chromosphere-corona transition region of the solar atmosphere
โ Scribed by O. V. Ptitsyna; B. V. Somov
- Book ID
- 111495498
- Publisher
- Allerton Press, Inc.
- Year
- 2010
- Tongue
- English
- Weight
- 194 KB
- Volume
- 65
- Category
- Article
- ISSN
- 0027-1349
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Qualitative arguments are presented to show that in the chromosphere-corona transition region the energy which is transported downwards by heat conduction cannot be disposed of by radiative losses only. The region therefore is unstable and forced to be in motion, which may give rise to spicule-like
Zentralinstitut fiir Astrophysik der Akadcmic der Wissenschaftcn der DDR Sonneiiol~servatoriuin Einsteintnrni IVitli 5 f i p r e s (Rcceivctl 1984 Sovembrr 30) Multiple wavelength observations of sunspot umbrae can only be expalined by an inhomogeneous, two-component model for the structure of the u